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作 者:Lorenzo Zaninetti Lorenzo Zaninetti(Physics Department, University of Turin, Turin, Italy)
机构地区:[1]Physics Department, University of Turin, Turin, Italy
出 处:《Journal of High Energy Physics, Gravitation and Cosmology》2024年第4期1538-1550,共13页高能物理(英文)
摘 要:We analyze a simple model for tired light in a cosmological environment, a generalized model, and a spectroscopic model. The three models are tested on different compilations for the distance modulus of supernovae. The tests are negative for the simple tired light and the spectroscopic models, but positive for the generalized tired light model. The percentage error of the distance modulus for the generalized tired light model compared with the distance modulus of standard cosmology is less than one percent over the considered ranges in redshift.We analyze a simple model for tired light in a cosmological environment, a generalized model, and a spectroscopic model. The three models are tested on different compilations for the distance modulus of supernovae. The tests are negative for the simple tired light and the spectroscopic models, but positive for the generalized tired light model. The percentage error of the distance modulus for the generalized tired light model compared with the distance modulus of standard cosmology is less than one percent over the considered ranges in redshift.
关 键 词:Galaxy Groups Large Scale Structure of the Universe Cosmology
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